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Exact critical bubble free energy and the effectiveness of effective potential approximations
Phys. Rev. D 49, 4094 – Published 15 April, 1994
DOI: https://doi.org/10.1103/PhysRevD.49.4094
Abstract
To calculate the temperature at which a first-order cosmological phase transition occurs, one must calculate , the free energy of a critical bubble configuration. is often approximated by the classical energy plus an integral over the bubble of the effective potential; one must choose a method for calculating the effective potential when . We test different effective potential approximations at one loop. The agreement is best if one pulls a factor into the decay rate prefactor [where ], and takes the real part of the effective potential in the region . We perform a similar analysis on the one-dimensional kink.
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